The Sydney-AAO Multi-object Integral field spectrograph

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The SAMI Galaxy Survey: the link between angular momentum and optical morphology The Integral Field View of the Orion Nebula The SAMI Galaxy Survey: asymmetry in gas kinematics and its links to stellar mass and star formation

P2860

Q58220720-DB815067-7741-4425-82EF-5AF5658BEB2E Q59035139-BF162122-1A92-44E8-9D8D-672BDE538986 Q59268291-840574BD-D6FF-4144-8B04-7981AD89307D

P2860

The Sydney-AAO Multi-object Integral field spectrograph

Item

http://www.wikidata.org/entity/Q59278806

description

im Februar 2012 veröffentlichter wissenschaftlicher Artikel

@de

wetenschappelijk artikel

@nl

наукова стаття, опублікована в лютому 2012

@uk

name

The Sydney-AAO Multi-object Integral field spectrograph

@en

The Sydney-AAO Multi-object Integral field spectrograph

@nl

type

Item

label

The Sydney-AAO Multi-object Integral field spectrograph

@en

The Sydney-AAO Multi-object Integral field spectrograph

@nl

prefLabel

The Sydney-AAO Multi-object Integral field spectrograph

@en

The Sydney-AAO Multi-object Integral field spectrograph

@nl

P1476

The Sydney-AAO Multi-object Integral field spectrograph

@en

P2093

Andrew M. Hopkins

http://www.w3.org/2001/XMLSchema#string

Christopher Trinh

http://www.w3.org/2001/XMLSchema#string

D. Heath Jones

http://www.w3.org/2001/XMLSchema#string

Holly Trowland

http://www.w3.org/2001/XMLSchema#string

Jon S. Lawrence

http://www.w3.org/2001/XMLSchema#string

Julia J. Bryant

http://www.w3.org/2001/XMLSchema#string

Lisa Fogarty

http://www.w3.org/2001/XMLSchema#string

Michael Goodwin

http://www.w3.org/2001/XMLSchema#string

Michael N. Birchall

http://www.w3.org/2001/XMLSchema#string

Ron Heald

http://www.w3.org/2001/XMLSchema#string

P2860

A Relationship between Nuclear Black Hole Mass and Galaxy Velocity Dispersion

Theoretical Modeling of Starburst Galaxies

New approach to atmospheric OH suppression using an aperiodic fibre Bragg grating.

Hexabundles: imaging fiber arrays for low-light astronomical applications.

Secular Evolution and the Formation of Pseudobulges in Disk Galaxies

Galaxy morphology in rich clusters - Implications for the formation and evolution of galaxies

A Fundamental Relation between Supermassive Black Holes and Their Host Galaxies

The Three-Phase Interstellar Medium Revisited

Astrophotonics: a new era for astronomical instruments.

The galactic abundance gradient

P304

no-no

http://www.w3.org/2001/XMLSchema#string

P31

scholarly article

P356

10.1111/J.1365-2966.2011.20365.X

http://www.w3.org/2001/XMLSchema#string

P407

English

P50

Samuel Nathan Richards

P577

2012-02-01T00:00:00Z

http://www.w3.org/2001/XMLSchema#dateTime

P818

1112.3367

http://www.w3.org/2001/XMLSchema#string

P819

2012MNRAS.421..872C

http://www.w3.org/2001/XMLSchema#string

The Sydney-AAO Multi-object Integral field spectrograph

about

sameAs

P2860

P2860

The Sydney-AAO Multi-object Integral field spectrograph

description

name

type

label

prefLabel

P1433

P1476

P2093

P2860

P304

P31

P356

P407

P50

P577

P818

P819

P356

P1433

P1476

P2093

P2860

P304

P31

P356

P407

P50

P577

P818

P819